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All types of supernovae (SNe), except Type Ia, have been observed to interact with their immediate circumstellar medium (CSM). This interaction can reveal their progenitor's histories, and constrain our ideas about the evolution of massive…

Astrophysics · Physics 2007-05-23 Robert J. Cumming , Peter Lundqvist

We derive new constraints on light CP-even scalars using old gamma-ray observations in the direction of SN1987A by the Solar Maximum Mission (SMM) satellite. Light scalars can be abundantly produced in the supernova core via the nucleon…

High Energy Physics - Phenomenology · Physics 2026-03-10 Yue Yu , Writasree Maitra , P. S. Bhupal Dev , Jean-Franccois Fortin , Steven P. Harris , Kuver Sinha , Yongchao Zhang

Axion-like particles (ALPs) are hypothetical pseudoscalar bosons that arise in many extensions of the Standard Model and are well-motivated dark matter candidates. Nearby massive stars in the late stages of stellar evolution provide a…

We present constraints on supernovae type Ia (SNe~Ia) progenitors through an analysis of the environments found at the explosion sites of 102 events within star-forming host galaxies. H-alpha and GALEX near-UV images are used to trace…

Astrophysics of Galaxies · Physics 2015-06-23 J. P. Anderson , P. A. James , F. Förster , S. González-Gaitán , S. M. Habergham , M. Hamuy , J. D. Lyman

The formation of a hot and dense core in a core-collapse supernova (SN) can produce massive Beyond Standard Model (BSM) particles. These particles can decay in the stellar envelope, generating positrons either directly or through secondary…

High Energy Physics - Phenomenology · Physics 2025-11-20 Garv Chauhan , Cecilia Lunardini

Studies of axion-like particles (ALPs) commonly focus on a single type of interaction, for example couplings only to photons. Most ALP models however predict correlations between different couplings, which change the phenomenology in…

High Energy Physics - Phenomenology · Physics 2020-07-15 Fatih Ertas , Felix Kahlhoefer

New feebly interacting particles would emerge from a supernova core with 100-MeV-range energies and produce $\gamma$-rays by subsequent decays. These would contribute to the diffuse cosmic $\gamma$-ray background or would have shown up in…

High Energy Physics - Phenomenology · Physics 2023-07-17 Melissa Diamond , Damiano F. G. Fiorillo , Gustavo Marques-Tavares , Edoardo Vitagliano

We provide a comprehensive analysis of the phenomenology of axion-like particles (ALPs) produced in core-collapse supernovae (ccSNe) through interactions with electrons and muons, both of which have a non-negligible abundance in the SN…

High Energy Physics - Phenomenology · Physics 2025-10-17 Ricardo Z. Ferreira , M. C. David Marsh , Eike Ravensburg

We carry out a comprehensive theoretical examination of the relationship between the spatial distribution of optical transients and the properties of their progenitor stars. By constructing analytic models of star-forming galaxies and the…

Astrophysics · Physics 2009-11-13 Cody Raskin , Evan Scannapieco , James Rhoads , Massimo Della Valle

Massive stars, possibly red supergiants, which retain extended hydrogen envelopes until core collapse, produce Type II Plateau (IIP) supernovae. The ejecta from these explosions shock the circumstellar matter originating from the mass loss…

High Energy Astrophysical Phenomena · Physics 2015-06-15 Sayan Chakraborti , Alak Ray , Randall Smith , Stuart Ryder , Naveen Yadav , Firoza Sutaria , Vikram V. Dwarkadas , Poonam Chandra , David Pooley , Rupak Roy

Axions or more generally axion-like particles (ALPs) are pseudo-scalar particles predicted by many extensions of the Standard Model of particle physics (SM) and considered as viable candidates for dark matter (DM) in the universe. If they…

High Energy Astrophysical Phenomena · Physics 2020-05-20 Ahmed Ayad , Geoff Beck

QCD axions would be copiously produced in the proto-neutron star formed in a core-collapse supernova (SN). After escaping, they would convert into gamma rays in the Galactic magnetic field and, as recently shown, in that of the progenitor…

High Energy Physics - Phenomenology · Physics 2026-05-06 Francisco R. Candón , Damiano F. G. Fiorillo , Ángel Gil Muyor , Hans-Thomas Janka , Georg G. Raffelt , Edoardo Vitagliano

Heavy sterile neutrinos can be produced in core-collapse supernovae (CCSNe), which are superb particle generators because of their high densities and temperatures. If the sterile neutrinos are long-lived, these may be produced inside the…

High Energy Physics - Phenomenology · Physics 2025-03-19 Garv Chauhan , R. Andrew Gustafson , Ian M. Shoemaker

In this article, we claim that axion-like particles (ALPs) with MeV masses can be produced with semi-relativistic velocities in core-collapse supernovae (SNe), generating a diffuse galactic flux. We show that these ALPs can be detected in…

High Energy Physics - Phenomenology · Physics 2025-07-15 David Alonso-González , David Cerdeño , Marina Cermeño , Andres D. Perez

The progenitors of low-luminosity Type II-Plateau supernovae (SNe II-P) are believed to be red supergiant (RSG) stars, but there is much disparity in the literature concerning their mass at core collapse and therefore on the main sequence.…

High Energy Astrophysical Phenomena · Physics 2017-12-06 Sergey M. Lisakov , Luc Dessart , D. John Hillier , Roni Waldman , Eli Livne

New pseudoscalars, axion-like particles (ALPs), provide the exciting target for present and future collider-based experiments. Search for ALPs is performed in this paper via the $W^{+}W^{-}$ fusion process…

High Energy Physics - Phenomenology · Physics 2023-12-08 Chong-Xing Yue , Han Wang , Yue-Qi Wang

Core collapse within blue supergiant stars, as occurred within Sk -69$^{\circ}$202/Supernova 1987A, is generally attributed to a merger of two electron-degenerate cores within a common envelope, with a merged mass in excess of 1.4 solar.…

High Energy Astrophysical Phenomena · Physics 2024-10-28 John Middleditch

We revisit SN1987A constraints on light, hidden sector gauge bosons ("dark photons") that are coupled to the standard model through kinetic mixing with the photon. These constraints are realized because excessive bremsstrahlung radiation of…

High Energy Physics - Phenomenology · Physics 2017-09-06 Cameron Mahoney , Adam K. Leibovich , Andrew R. Zentner

We consider the constraints from Supernova 1987A on particles with small couplings to the Standard Model. We discuss a model with a fermion coupled to a dark photon, with various mass relations in the dark sector; millicharged particles;…

High Energy Physics - Phenomenology · Physics 2018-09-18 Jae Hyeok Chang , Rouven Essig , Samuel D. McDermott

We have attempted to constrain the progenitors of all supernova types, through correlations of the positions of historical supernovae with recent star formation, as traced by H-alpha emission. Through pixel statistics we have found that a…

Astrophysics · Physics 2009-06-23 J. P. Anderson , P. A. James , M. Salaris , S. M. Percival